About: Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys     Goto   Sponge   NotDistinct   Permalink

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  • In this article, we present results based on high-density, high-precision Wide-Angle Search for Planets (WASP) light curves supplemented with lower-precision photometry from the All-Sky Automated Survey (ASAS) for 268 RR Lyrae stars (176 regular, 92 Blazhko). Light curves were Fourier-decomposed and coefficients from WASP were transformed to the ASAS standard using 24 common stars. Coefficients were then compared with similar data from Galactic globular clusters, the Galactic bulge and the Large and Small Magellanic Clouds (LMC and SMC). Using Fourier coefficients, we also calculated physical parameters via standard equations from the literature. We confirmed the results of previous authors, including lower amplitudes and longer rise times for Blazhko stars. It was found that in the R31 versus R21 plot the location of a star depends mainly on its metallicity and that Blazhko stars prefer a different location from modulation-free stars.
  • In this article, we present results based on high-density, high-precision Wide-Angle Search for Planets (WASP) light curves supplemented with lower-precision photometry from the All-Sky Automated Survey (ASAS) for 268 RR Lyrae stars (176 regular, 92 Blazhko). Light curves were Fourier-decomposed and coefficients from WASP were transformed to the ASAS standard using 24 common stars. Coefficients were then compared with similar data from Galactic globular clusters, the Galactic bulge and the Large and Small Magellanic Clouds (LMC and SMC). Using Fourier coefficients, we also calculated physical parameters via standard equations from the literature. We confirmed the results of previous authors, including lower amplitudes and longer rise times for Blazhko stars. It was found that in the R31 versus R21 plot the location of a star depends mainly on its metallicity and that Blazhko stars prefer a different location from modulation-free stars. (en)
Title
  • Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys
  • Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys (en)
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  • Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys
  • Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys (en)
skos:notation
  • RIV/00216224:14310/14:00077141!RIV15-MSM-14310___
http://linked.open...avai/riv/aktivita
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  • S
http://linked.open...iv/cisloPeriodika
  • 2
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http://linked.open...aciTvurceVysledku
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  • 6903
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  • RIV/00216224:14310/14:00077141
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  • methods: data analysis; techniques: photometric; stars: horizontal branch; stars: variables: RR Lyrae (en)
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  • GB - Spojené království Velké Británie a Severního Irska
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  • [C33F1A47C512]
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  • Monthly Notices of the Royal Astronomical Society
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http://linked.open...v/svazekPeriodika
  • 445
http://linked.open...iv/tvurceVysledku
  • Skarka, Marek
http://linked.open...ain/vavai/riv/wos
  • 000346959400044
issn
  • 0035-8711
number of pages
http://bibframe.org/vocab/doi
  • 10.1093/mnras/stu1815
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  • 14310
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